Discrete Newtonian Gravitation and the Three-Body Problem

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dc.contributor.authorGreenspan, Donalden_US
dc.date.accessioned2012-03-15T16:20:42Z
dc.date.available2012-03-15T16:20:42Z
dc.date.created1971en_US
dc.date.issued1971en
dc.description.abstractNewtonian gravitation is studied from a discrete point of view in that the dynamical equation is an energy conserving difference equation. Application is made to planetary type, nondegenerate three-body problems and several computer examples of perturbed orbits are given.en_US
dc.format.mimetypeapplication/pdfen_US
dc.identifier.citationTR133en
dc.identifier.urihttp://digital.library.wisc.edu/1793/57714
dc.publisherUniversity of Wisconsin-Madison Department of Computer Sciencesen_US
dc.titleDiscrete Newtonian Gravitation and the Three-Body Problemen_US
dc.typeTechnical Reporten_US

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